Stellar Turbulence [E-Book] : Proceedings of Colloquium 51 of the International Astronomical Union Held at the Universtiy of Western Ontario London, Ontario, Canada August 27–30, 1979 / edited by David F. Gray, Jeffery L. Linsky.
Saved in:
Full text |
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Personal Name(s): | Gray, David F., editor |
Linsky, Jeffery L., editor | |
Imprint: |
Berlin, Heidelberg :
Springer,
1980
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Physical Description: |
online resource. |
Note: |
englisch |
ISBN: |
9783540385547 |
DOI: |
10.1007/3-540-09737-6 |
Series Title: |
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Lecture Notes in Physics ;
114 |
Subject (LOC): |
- Stellar convection theory
- Instabilities in a polytropic atmosphere
- On the dynamics of the solar convection zone
- Thermal and continuum driven convection in B-stars
- The height dependence of granular motion
- Numerical simulation of the solar granulation
- Differential rotation in stars with convection zones
- Generation of oscillatory motions in the stellar atmosphere
- The evolution of an average solar granule
- Observed solar spectral line asymmetries and wavelength shifts due to convection
- Differential line shifts in late type stars
- Temporal and spatial fluctuations in widths of solar EUV lines
- Formation of the profiles of absorption lines in the inhomogeneous medium
- The determination of stellar turbulence by low resolution techniques
- Analysis of high resolution stellar line profiles
- Examples of non-thermal motions as seen on the sun
- Diagnostic use of FE II H & K wing emission lines
- Turbulence in main sequence stars
- Observational aspects of macroturbulence in early type stars
- Photospheric Macroturbulence in late-type stars
- Depth-dependence of turbulence in stellar atmospheres
- Turbulence in the atmospheres of eclipsing binary stars
- Differential line-shifts
- Time dependence of Balmer progression in the spectrum of HD 92207
- Microturbulence : Age dependences
- High luminosity F-K stars motions and H? emissions
- Turbulence in the atmosphere of B-type starsmissions
- Mesoturbulence
- Stochastic approach
- The application of mesoturbulence to stellar atmospheres
- Effects of acoustic waves on spectral line profiles
- Some effects of strong acoustic waves on strong spectral lines
- Numerical simulation of granular convection: Effects on photospheric spectral line profiles
- Mechanical energy transport
- Stellar chromospheres
- Observations of the outer atmospheric regions of ? Orionis
- Stellar-winds and coronas in cool stars
- Relationship between envelope structure and energy source of non-thermal motions
- An analysis of microturbulence in the atmosphere of the F-type supergiant gamma cygni
- The solar chromospheric microturbulence and the emission observed at eclipse
- Excitation dependent gf-values and depth dependent microturbulences
- On the structural and stochastic motions in the solar and stellar atmospheres
- I U E observations of circumstellar lines and mass loss from B-star
- On the establishment of internally consistent abundance-oscillator strength scales
- Differential rotation and magnetic activity of the lower main sequence stars
- Changes of photospheric line asymmetries with effective temperature
- Small-scale versus large scale motions in the solar atmosphere derived from a non-LTE calculation of multiplet 38 of Ti I
- Effects of flux tubes on conventional chromospheric diagnostics
- Summary.